Posts Tagged ‘nasa’

New comet discovered- may become one of the brightest in history……. until a brighter one comes along

October 8, 2012
Comet Lovejoy picture: people watching the comet from Perth, Australia

Sky-watchers in Australia ogle comet Lovejoy late last year.

Photograph by John Goldsmith, TWAN

Andrew Fazekas

for National Geographic News

Published September 27, 2012

If astronomers’ early predictions hold true, the holidays next year may hold a glowing gift for stargazersa superbright comet, just discovered streaking near Saturn.

Even with powerful telescopes, comet 2012 S1 (ISON) is now just a faint glow in the constellation Cancer. But the ball of ice and rocks might become visible to the naked eye for a few months in late 2013 and early 2014—perhaps outshining the moon, astronomers say.

The comet is already remarkably bright, given how far it is from the sun, astronomer Raminder Singh Samra said. What’s more, 2012 S1 seems to be following the path of the Great Comet of 1680, considered one of the most spectacular ever seen from Earth.

“If it lives up to expectations, this comet may be one of the brightest in history,” said Samra, of the H.R. MacMillan Space Centre in Vancouver, Canada.

So what makes a comet a showstopper? A lot depends on how much gas and dust is blasted off the central core of ice and rocks. The bigger the resulting cloud and tail, the more reflective the body may be.

Because 2012 S1 appears to be fairly large—possibly approaching two miles (three kilometers) wide—and will fly very close to the sun, astronomers have calculated that the comet may shine brighter, though not bigger, than the full moon in the evening sky.

(Also see “New Comet Found; May Be Visible From Earth in 2013.”)

Refugee From the Edge of the Solar System?

First spotted late last week by Russian astronomers Artyom Novichonok and Vitali Nevski of the International Scientific Optical Network (ISON), comet 2012 S1 was confirmed by the International Astronomical Union on Monday.

But while we know what 2012 S1 is, it’s still unclear where it came from. Its orbit suggests the comet may be a runaway from the Oort cloud, where billions of comets orbit about a hundred thousand times farther from the sun than Earth is.

“For astronomers, these distant origins are exciting,” Samra said, “because it allows us to study one of the oldest objects in the solar system still in its original, pristine condition.”

(Related: “Comet Is Cosmic Snow Globe, NASA Flyby Shows.”)

New Comet Bound for Glory?

Right now, 2012 S1 appears to be about 615 million miles (990 million kilometers) from Earth, between the orbits of Saturn and Jupiter, astronomers say.

As the sun’s gravity pulls the comet closer, it should pass about 6.2 million miles (10 million kilometers) from Mars—possibly a unique photo opportunity for NASA’s new Curiosity rover.

Current orbital predictions indicate the comet will look brightest to us in the weeks just after its closest approach to the sun, on November 28, 2013—if 2012 S1 survives the experience.

As the comet comes within about 1.2 million miles (2 million kilometers) of the sun, the star’s intense heat and gravity could cause the ice and rubble to break apart, scotching the sky show. (Related: “Comet Seen Vaporizing in Sun’s Atmosphere—A First.”)

“While some predictions suggest it may become as bright as the full moon, and even visible during the day, one should be cautious when predicting how exciting a comet may get,” Samra said.

“Some comets have been notorious for creating a buzz but failing to put on a dazzling display,” he said. “Only time will tell.”

More: See the first pictures of a peanut-like comet >>

so get out your cameras and tripods and stand by or you could read david hobby’s the strobist about jonathan snyder’s  So- Cool- It- Must- Be-Fake night portrait and see how it’s done.

jene

Space; the final frontier, now where have i heard that before

May 23, 2012

i’ve always found space and NASA space pictures interesting. i know nothing about astronomy nor physics but the concept of where we really live amazes me. as does all these inner workings of our bodies because it’s all done in the dark where the only thing i seem to be good at is stubbing my toes.

but thanks to Discovery magazine and Phil Plait of Bad Astronomy i can learn something or at least look at pretty cool pictures.

these are the type of pictures i ‘d like to show at Winkel & Balkticks  upcoming lab gathering but so far not received a response from them, there is a meeting tomorrow night thursday in Brooklyn to talk about the event. 135 Plymouth St, 208, Brooklyn @ 7:30

today the space i will be looking at is the inside of my epson 7600 printer to clear a clogged head. maybe i’ll learn something new besides a few curse word phrases. it’s a grey day out so why not give it a whirl. sounds like fun huh? well after spending weeks getting two exhibits together one at annex 24 in lancaster, pa the other one here in nyc at kahve , 774 9th ave, nyc, ny i am a bit worn out of framing stuff.

the latter is part of hell’s kitchen artist studio tour which seems to be about parties as they have an opening one fri another one sun night. oh well lots of performers living in the neighborhood. this can be a very confusing event because of the all volunteer nature of the event also the president of hka.org is a bit disorganized although he means well. i am not a party person per say so i stayed home enjoying working on the house. i do enjoy stepping back and seeing something substantial for my efforts.

BTW here is a link for my portfolio at ‘Art Takes Times Square’ that i would appreciate my readers to click through, thank you click on Collect me button on top, it doesn’t cost anything to become a judge.

    • Use the tools available to you. A suite of sharing tools is conveniently accessible right from your portfolio page. Just click on the ‘Share’ button located near the top right corner of your portfolio to see all your options. Start with the basics (Facebook, Twitter, Tumblr and Email), then take advantage of as many additional options as you can to maximize your visibility! You can also post your portfolio link on our Facebook page to share with the 80,000 people who like us. 🙂
    • Tap into your network. Share your work with as many people as you can. Have you encouraged friends, family members and colleagues to collect your work? Are you part of a club or community? Share your portfolio and encourage your fans to help you out by passing along your work to their networks!
  • Time Management. Remember that you have until this Friday May 25th Midnight EST to get into as many collections as you can. The sooner they collect you, the closer you are to winning Art Takes Times Square.

Andromeda’s majestic spray of billions of hot stars

Well, what can I say about this devastating and jaw-dropping picture of our nearest spiral neighbor, the Andromeda Galaxy?

[Click to massive chainedmaidenate. Do it!]

Well, I could start with HOLY HALEAKALA!

This image is a collection of 11 separate observations of Andromeda taken by NASA’s GALEX satellite. Launched in 2003, GALEX (which stands for Galaxy Evolution Explorer) scans the sky in ultraviolet light, specifically targeting galaxies. Hot stars produce UV light, and so does the gas it illuminates, so by looking in the ultraviolet astronomers can learn about how galaxies are constructed. In the decade since its launch, GALEX has been phenomenally successful, cataloging hundreds of millions of galaxies, some as far as ten billion light years away!

This image of Andromeda is simply stunning. It’s comprised of two colors: what you see here as blue is higher-energy ultraviolet light, and red is lower energy (closer to the kind of light we see). Right away you can see that objects emitting the higher-energy UV are confined to the spiral arms, and lower-energy emitters are spread out across the galaxy. That’s exactly what I would expect: massive stars, the kind that really blast out UV, don’t live very long. They’re born, live out their short lives, and die (as supernovae) pretty much near the spot where they formed, which is in spiral arms. Lower mass stars live long enough to gradually move away from their nurseries, populating the rest of the galaxy.

Also, star formation at the very center of the galaxy probably occurred long ago and shut down, so we don’t see many or any massive stars there.

One thing I didn’t know is that the arms of Andromeda are more like rings! The galaxy is at such a narrow angle that it’s hard to tell, but if you trace the blue emission, the pattern does look more like a ring than a spiral. This jibes with earlier images in infrared taken by Spitzer Space Telescope (which I’ve inset here) and a huge and incredibly beautiful newer one taken with ESA’s Herschel far-infrared telescope (and OMFSM you want to click that link).

From what I’ve read, it’s not clear why the spiral arms appear to be more ring-like. Which I love. Why? Because Andromeda is the nearest big spiral galaxy in the sky, a mere 2.5 or so million light years away. It’s easily visible to the naked eye from a dark site, and I’ve seen it myself countless times using my own eyes, binoculars, and telescopes ranging from small ones up to Hubble. Yet there it is, in all its huge and obvious splendor and beauty, still able to surprise me. That rocks.

And a note about GALEX: NASA recently handed off its operations to Caltech, a very unusual move. The satellite was put into standby mode in February, and I was worried it would be shut down permanently. However, Caltech signed a three-year agreement with NASA — while NASA still owns the satellite, Caltech will now be in control of GALEX’s science mission, managing and operating it. At the end of the agreement it can be renegotiated if GALEX is still in good operating condition. This is an interesting idea, and I’m not sure how I feel about it. I love that GALEX gets to continue operations, but handing off science missions to private groups makes me a little uneasy. In this particular case I think it’s fine — Caltech is a research institute after all — but the precedent may have unforeseen consequences. We’ll see.

Still and all, it’s good to see new life breathed into an important and wonderful instrument like GALEX. I certainly hope it will continue to produce cutting-edge science for years to come… as well as amazingly beautiful images like this one.

Image credit: NASA/JPL-Caltech